Do we have much sub-surface data from the Galp & Rhino blocks? (i've not seen much floating around publically) - it would be useful to compare & contrast with what we know about Saturn - ie, we share same source rock, avo 2 & 3 anomolies seem proven, kudu source kitchen, east of outer high seems to have higher permeabilities & porosities, etc, etc). It seems generally acknowledged that there is some geological complexity in the saturn block (from various sources); but the same has been said about the Galp block (with up to 3 seperate reservoirs so far). The more 'nearology' success we have, certainly the more it derisks further exploration, and should lead to better GCOS for saturn (I'm in agrement on that one). Interesting times ahead.
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